The result is shown in Fig. REF . Although with fully efficient
circulation (\(\alpha =1/4\) ) the geometric albedo can be as high as
\(A_g=0.43\pm 0.15\) , based on the Ks occultation data
[1]} and several other, more direct studies
[2]}
it is highly unlikely that WASP-5 b stands out from the other hot
Jupiters, that mostly have low circulation efficiency. Therefore,
it is quite reasonable to assume that the true value of \(A_g\)  is
closer to the no circulation limit of \(A_g=0.29 \pm 0.15\) .
